Red-burning galaxies hold the key to galaxy evolution

Figure 1: A panoramic view of the CL0939+4713 cluster located 4 billion light years away from Earth. Images were captured with the Subaru Prime Focus Camera (Suprime-Cam), all of which are a composite of a B-band image (blue), a R-band image (green), and a z'-band image (red). Left 27 arcmin x 27 arcmin field of view.
Top-right: Close-up view of the central cluster region, 2.5 arcmin x 2.5 arcmin field of view.
Bottom-right:Example of the concentration of red-burning galaxies, which are marked with red squares.

Figure 1: A panoramic view of the CL0939+4713 cluster located 4 billion light years away from Earth. Images were captured with the Subaru Prime Focus Camera (Suprime-Cam), all of which are a composite of a B-band image (blue), a R-band image (green), and a z'-band image (red). Left 27 arcmin x 27 arcmin field of view.
Top-right: Close-up view of the central cluster region, 2.5 arcmin x 2.5 arcmin field of view.
Bottom-right:Example of the concentration of red-burning galaxies, which are marked with red squares.

A research team of astronomers from the University of Tokyo and the National Astronomical Society of Japan (NAOJ) has identified the location of red star-forming galaxies around a galaxy cluster situated four billion light years distant from Earth. A panoramic observation with the Subaru Telescope yielded the result. Scientists surmise that such "red-burning galaxies" are in a transitional phase from a young generation of galaxies to older one; they may demonstrate the dramatic evolution of galaxies in the environment surrounding the cluster.

The key areas for understanding how environment shaped galaxy evolution in the past universe may be where red-burning galaxies are most numerous, in small groups on the outskirts of the rich cluster rather than within it.

The birth of galaxies occurred more than ten billion years ago in the ancient Universe. Assembled under their own gravity, early galaxies formed into big clusters or small groups. During the process of assemblage, their properties changed in relation to their surrounding environments, just as human traits change in the contexts of their lives. For example, galaxies grouped in high-density environments such as clusters tend to be elliptical or lenticular while solitary ones tend to be spiral galaxies. How galaxies form and evolve is one of the biggest mysteries in recent extragalactic astronomy.

Figure 2: An image illustrating the number density of galaxies estimated to be four billion light years from the Earth. Bright areas indicate high-density regions. The brightest region in the center corresponds to the main body of the CL0939 cluster. Red squares show the positions of the red -burning galaxies while the greenish-blue dots show the blue Hα emitting galaxies. Evidently, the red burning galaxies avoid the central region of the cluster and concentrate in small groups located far away from it.

When and how did patterns of galactic formation become established and evolve? To address this question, many astronomers are investigating distant clusters of galaxies where assemblage of galaxies occurred in the early universe. A research team led by Dr. Yusei Koyama used the Subaru Prime Focus Camera (Suprime-Cam) to carry out a panoramic observation targeting a relatively well-known rich cluster, CL0939+4713, located four billion light years away from Earth (see Fig. 1). The team used a special filter that can detect the hydrogen-alpha (Hα) line emitted by ionized hydrogen four billion years ago . Koyama's team members carefully compared the images taken with and without the special filter and then identified more than 400 galaxies showing an excess of Hα in the special filter images (see Fig. 2). Such narrow-band "excess" galaxies are likely to be star-forming galaxies. Surprisingly, Koyama's team found that an unexpectedly large number of star-forming galaxies had red colors. Even more interesting was the location of these red-burning galaxies; they reside primarily in the group-scale environments located far away from the main body of the cluster .

These findings raise some intriguing questions. What is the physical origin of these red-burning galaxies? Why are they concentrated in groups and not in clusters? No one, including the research team members, knows the answer yet. At a minimum, the strong Hα emissions clearly show that the red-burning galaxies are actively forming new stars. Therefore, their red colors are likely to be produced by dust rather than by old stellar populations. The researchers expect that the strong gravity of the main cluster will cause the groups where the red-burning galaxies are most numerous to merge with it. The most significant result of this research is that the properties of galaxies are indeed changing in relatively sparse environments before they are finally absorbed into a very rich cluster.

The research team noticed that the number of old galaxies, without active star-formation, appeared to be increasing in the group environments, exactly where the red-burning galaxies are most numerous. This suggests that the red-burning galaxies are related to the increase in old galaxies, and that they are likely to be in a transitional phase from a younger to an older generation. The finding that such transitional galaxies are located most frequently within group environments shows that galaxy groups are the key environments for understanding how environment shapes the evolution of galaxies.

The research team emphasized the important contribution of the unique wide-field capability of the Subaru Telescope for accomplishing this research, because its panoramic imaging revealed the location of the transitional galaxies. The same research team now plans to conduct a new observation to identify the physical origin of the red-burning galaxies discovered in this study. This should be an important and exciting step toward a more complete understanding of the environments shaping the galaxies in the present-day universe.